In [1]} the local BRST cohomology was computed for old [2]}, [3]} and new [4]} minimal supergravity, both for pure supergravity and for supergravity coupled to matter multiplets (Yang-Mills multiplets and chiral matter multiplets). The results for candidate anomalies are summarized in section 9 of [1]}. Ten different types of candidate anomalies were found, denoted by type I, II, III, IVa, IVb and Va to Ve, cf. table 9.1 of [1]}. The candidate anomalies of type III, IVb, Vc, Vd and Ve occur only in new minimal supergravity because they are related to the presence of a 2-form gauge potential in the supergravity multiplet of new minimal supergravity and thus do provide a candidate that could be equivalent to (REF ).
The candidate anomalies of type I, IVa, Va and Vb each involve at least two different Yang-Mills gauge fields and thus neither provide a candidate that could be equivalent to (REF ).
